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Title: Growth of the Rayleigh{endash}Taylor instability in an imploding Z-pinch

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.872168· OSTI ID:467310
;  [1];  [2];  [2]
  1. Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
  2. Department of Physics, Uppsala University, Box 530, S-751 21, Uppsala (Sweden)

Rayleigh{endash}Taylor (RT) instability of cylindrical, imploding plasma liners in a Z-pinch is analyzed. The reduction in total perturbation growth for multicascade systems (multiple imploding shells) is presented. This reduction is effective if the pressure produced by the impacting shell exceeds the magnetic pressure at the time of impact. Analytical and numerical solutions are also obtained for the RT instability of an imploding plasma liner accelerated into undisturbed plasma. The snowplow model is used in which the mass encountered by the imploding magnetic piston is swept into an infinitely thin sheath. A shock front launched ahead of the liner is shown to reduce the growth rate. It is also shown that accumulating the mass increases the growth rate. However, the total perturbation growth can be reduced if the liner accumulates the mass during the implosion compared to a liner with the same mass imploding into vacuum. Finally, it is shown that the final kinetic energy density for a given shell nonuniformity is largest if the final liner mass is accumulated during the implosion. {copyright} {ital 1997 American Institute of Physics.}

Research Organization:
Sandia National Laboratories (SNL), Albuquerque, NM, and Livermore, CA (United States)
DOE Contract Number:
AC04-94AL85000
OSTI ID:
467310
Journal Information:
Physics of Plasmas, Vol. 4, Issue 3; Other Information: PBD: Mar 1997
Country of Publication:
United States
Language:
English